Global Monitoring of the Terrestrial Ring Current - ESA Space ...

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H O He H (O) [Liemohn et al., JGR, 106, 10883, 2001] Alpbach Summer School, 2002 Energy density pr<strong>of</strong>iles (proportional to plasma pressure) Alpbach Summer School, 2002
ASTRID (SAC-B) CASSINI PROCESSES INVESTIGATED VIA ENA Remote sensing <strong>of</strong>: Magnetized bodies (Earth, Mercury, Jupiter, Saturn…) Magnetospheric Plasma IMAGE Circulation Charge exchange! Non-magnetized bodies with MARS atmosphere EXPRESS (Mars, Venus…) Solar wind-induced neutral gas escape Charge exchange & sputtering! Bodies without atmosphere (Mercury, Moon, Asteroids…) TWINS Solar wind-induced surface erosion Sputtering! The Sun Solar wind acceleration region Neutral solar wind! VENUS EXPRESS BEPICOLOMBO SOLAR ORBITER Alpbach Summer School, 2002 ENA precipitating at low altitudes Alpbach Summer School, 2002
Page 1 and 2: Global Monitoring of the Terrestria
Page 3 and 4: Alpbach Summer School, 2002 gyratio
Page 5 and 6: Alpbach Summer School, 2002 Conside
Page 7 and 8: Ring Current sources Inward transp
Page 9 and 10: [Ebihara and Ejiri, JGR,105, 15843,
Page 11: Model inputs H + data from geosynch
Page 15 and 16: Alpbach Summer School, 2002 ENA flu
Page 17 and 18: Alpbach Summer School, 2002 Alpbach
Page 19 and 20: (fm fm.: .: D. Mitchell et al., Yos
Page 21 and 22: IMAGE Era Accomplishments in Substo
Page 23 and 24: Model validation. Comparison of the
Page 25 and 26: Modeled Storm Time Evolution Of Equ
Page 27 and 28: Alpbach Summer School, 2002 H + Flu
Page 29 and 30: Alpbach Summer School, 2002 Modeled
Page 31 and 32: ∞ ∫ 0 Alpbach Summer School, 20
Page 33 and 34: ε = 1 2 Alpbach Summer School, 200
Page 35 and 36: Alpbach Summer School, 2002 SUMMARY
Page 37: [Ebihara and Ejiri, JGR,105, 15843,

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